-
Notifications
You must be signed in to change notification settings - Fork 0
Commit
This commit does not belong to any branch on this repository, and may belong to a fork outside of the repository.
- Loading branch information
Showing
13 changed files
with
25 additions
and
25 deletions.
There are no files selected for viewing
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
Original file line number | Diff line number | Diff line change |
---|---|---|
@@ -1 +1 @@ | ||
blue compact dwarf galaxies, red-giant stars, interstellar gas, metagalactic UV background, superwinds; determine star formation history of blue compact dwarf galaxies, understand the faint blue excess, study the delayed formation of dwarfs, analyze the effects of starburst feedback on the interstellar medium, provide a unique laboratory for low-mass system evolution | ||
isolated dwarf galaxies, WLM, Pegasus Dwarf Irregular Galaxy, stellar mass, main sequence stars; understand growth of stellar mass in WLM and PegDIG, constrain effects of reionization, analyze radial population gradients, study variable star populations in WLM and PegDIG |
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
Original file line number | Diff line number | Diff line change |
---|---|---|
@@ -1 +1 @@ | ||
short-duration gamma-ray bursts, kilonova, neutron star material, radioactive transients, r-process elements; directly support compact object merger hypothesis for short-duration GRBs, provide new electromagnetic localization signature for gravitational wave sources, suggest kilonovae as likely sites of r-process element production, inform searches of gravitational wave error boxes, quantify contribution to heavy element nucleosynthesis budget | ||
supernova SN 1987A, circumstellar ring, supernova remnant, shocked ring, radioactive isotopes; determine mass loss of Sanduleak -69 202 progenitor, test ideas for SN 1987A progenitor, analyze shape of SN 1987A explosion, resolve inner debris of SN 1987A, reveal true extent of gas outside the ring |
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
Original file line number | Diff line number | Diff line change |
---|---|---|
@@ -1 +1 @@ | ||
compact galaxy groups, star formation regions, young and old star clusters, tidal features, active galactic nuclei, intragroup gas, Spitzer-identified regions; study stellar nurseries in compact groups, analyze kinematics of intragroup gas, detect and classify active galactic nuclei, compare properties of young and old star clusters, identify and categorize tidal features in compact groups | ||
X-ray luminous galaxy clusters, eMACS clusters, Balmer Break Galaxies, Lyman-break galaxies, gravitational telescopes; identify most powerful gravitational telescopes for future studies, constrain mass distribution within extreme systems, improve understanding of galaxy-galaxy and galaxy-gas interactions, unveil Balmer Break Galaxies at z~2, detect Lyman-break galaxies at z>6 |
Binary file not shown.
Binary file not shown.
Binary file not shown.
Binary file not shown.
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
Original file line number | Diff line number | Diff line change |
---|---|---|
@@ -1,4 +1,4 @@ | ||
1. irregular galaxies | ||
2. barred spiral galaxies | ||
3. Cepheid variables | ||
4. dwarf galaxies | ||
1. dwarf galaxies | ||
2. RR Lyrae variables | ||
3. red giants | ||
4. trans-Neptunian objects |
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
Original file line number | Diff line number | Diff line change |
---|---|---|
@@ -1,4 +1,4 @@ | ||
1. jets and outflows | ||
2. first galaxies | ||
3. black holes | ||
4. dark energy | ||
1. supernova remnants | ||
2. protostars | ||
3. galactic structure | ||
4. core-collapse supernova |
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
Original file line number | Diff line number | Diff line change |
---|---|---|
@@ -1,4 +1,4 @@ | ||
1. first galaxies | ||
2. black holes | ||
3. galaxy archeology | ||
4. galaxy evolution | ||
1. galaxy clusters | ||
2. lyman alpha | ||
3. intracluster medium | ||
4. dark energy |
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
Original file line number | Diff line number | Diff line change |
---|---|---|
@@ -1,4 +1,4 @@ | ||
1. dwarf galaxies | ||
2. globular clusters | ||
1. high-redshift quasars | ||
2. gravitational lensing | ||
3. low surface brightness galaxies | ||
4. ultra diffuse galaxies | ||
4. white dwarfs |
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
Original file line number | Diff line number | Diff line change |
---|---|---|
@@ -1,4 +1,4 @@ | ||
1. supernovae | ||
2. high-redshift quasars | ||
3. gravitational lensing | ||
4. ultra diffuse galaxies | ||
1. gravitational lensing | ||
2. supernovae | ||
3. binary star systems | ||
4. circumstellar disks |
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
Original file line number | Diff line number | Diff line change |
---|---|---|
@@ -1,4 +1,4 @@ | ||
1. gravitational lensing | ||
2. Kuiper Belt objects | ||
3. gamma-ray bursts | ||
4. high-redshift quasars | ||
2. high-redshift quasars | ||
3. ultra diffuse galaxies | ||
4. galaxy clusters |